HE 1523-0901: Difference between revisions
比利时188393热度 (talk | contribs) No edit summary Tag: Reverted |
No edit summary Tags: Manual revert Reverted |
||
| Line 16: | Line 16: | ||
{{Starbox character |
{{Starbox character |
||
| type = [[red giant branch]]<ref name=dr3/> |
| type = [[red giant branch]]<ref name=dr3/> |
||
| class = |
| class = [[CEMP star|CEMP]]<ref name=placco2018>{{cite journal |bibcode=2018AJ....155..256P |title=Spectroscopic Validation of Low-metallicity Stars from RAVE |last1=Placco |first1=Vinicius M. |last2=Beers |first2=Timothy C. |last3=Santucci |first3=Rafael M. |last4=Chanamé |first4=Julio |last5=Sepúlveda |first5=María Paz |last6=Coronado |first6=Johanna |last7=Points |first7=Sean D. |last8=Kaleida |first8=Catherine C. |last9=Rossi |first9=Silvia |last10=Kordopatis |first10=Georges |last11=Lee |first11=Young Sun |last12=Matijevič |first12=Gal |last13=Frebel |first13=Anna |last14=Hansen |first14=Terese T. |last15=Holmbeck |first15=Erika M. |last16=Rasmussen |first16=Kaitlin C. |last17=Roederer |first17=Ian U. |last18=Sakari |first18=Charli M. |last19=Whitten |first19=Devin D. |journal=The Astronomical Journal |year=2018 |volume=155 |issue=6 |page=256 |doi=10.3847/1538-3881/aac20c |arxiv=1805.00608 |s2cid=119460225 |doi-access=free }}</ref> |
||
| b-v = +1.057<ref name=ubv/> |
| b-v = +1.057<ref name=ubv/> |
||
}} |
}} |
||
| Line 27: | Line 27: | ||
| dist_ly= |
| dist_ly= |
||
| dist_pc= |
| dist_pc= |
||
| absmag_v = |
| absmag_v = |
||
}} |
}} |
||
{{Starbox detail |
{{Starbox detail |
||
| Line 42: | Line 42: | ||
}} |
}} |
||
{{Starbox end}} |
{{Starbox end}} |
||
'''HE 1523-0901''' is the designation given to a [[ |
'''HE 1523-0901''' is the designation given to a [[red giant]] [[star]] in the [[Milky Way]] galaxy approximately 9,900 [[light year]]s from [[Earth]]. It is thought to be a [[Stellar population|second generation]], [[Population II]], or metal-poor, star ([Fe/H] = −2.95). The star was found in the sample of bright metal-poor [[halo star]]s from the [[Hamburg/ESO Survey]] by [[Anna Frebel]] and collaborators. The group's research was published in the May 10, 2007 issue of ''[[The Astrophysical Journal]]''.<ref name="frebel"> |
||
{{cite journal |
{{cite journal |
||
|last1= Frebel|first1=A. |
|last1= Frebel|first1=A. |
||
| Line 85: | Line 85: | ||
[[Category:Giant stars]] |
[[Category:Giant stars]] |
||
[[Category:Population II stars]] |
[[Category:Population II stars]] |
||
[[Category:G-type hypergiants]] |
|||
Revision as of 13:58, 19 January 2024
 | This article includes a list of general references, but it lacks sufficient corresponding inline citations. (July 2023) |
 Artist's impression of HE 1523-0901 | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Libra |
| Right ascension | 15h 26m 01.070s[1] |
| Declination | −9° 11′ 38.89″[1] |
| Apparent magnitude (V) | 11.129[2] |
| Characteristics | |
| Evolutionary stage | red giant branch[1] |
| Spectral type | CEMP[3] |
| B−V color index | +1.057[2] |
| Astrometry | |
| Proper motion (μ) | RA: −22.685[1] mas/yr Dec.: −28.204[1] mas/yr |
| Parallax (π) | 0.3278 ± 0.0140 mas[1] |
| Distance | 9,900 ± 400 ly (3,100 ± 100 pc) |
| Details | |
| Mass | 27[4] M☉ |
| Radius | 730[1] R☉ |
| Luminosity | 243,000 [1] L☉ |
| Surface gravity (log g) | 1.29[4] cgs |
| Temperature | 4,742[4] K |
| Metallicity [Fe/H] | −2.65[4] dex |
| Age | 13.2[5] Gyr |
| Database references | |
| SIMBAD | data |
HE 1523-0901 is the designation given to a red giant star in the Milky Way galaxy approximately 9,900 light years from Earth. It is thought to be a second generation, Population II, or metal-poor, star ([Fe/H] = −2.95). The star was found in the sample of bright metal-poor halo stars from the Hamburg/ESO Survey by Anna Frebel and collaborators. The group's research was published in the May 10, 2007 issue of The Astrophysical Journal.[5]
Age
The star's age, as measured by ESO's Very Large Telescope, is 13.2 billion years. This makes it among the oldest stars[6] and nearly as old as the estimated age of the universe itself (13.8 billion years as measured by Planck). The measurement uncertainty in the age estimate is 0.7 to 2.7 billion years, depending upon the assumptions made to estimate the uncertainty, although the uncertainty in the relative age of this and other stars using the same method is smaller.[5] HE 1523-0901 is the first star whose age was determined using the decay of the radioactive elements uranium and thorium in tandem with measurements of several neutron capture elements.[7] It is believed to have formed directly from the remnants of the first-generation stars that reached the end of their longevity and exploded as supernovae early in the history of known matter.
Designation
The designation "HE 1523-0901" indicates that the star is part of the Hamburg/ESO Survey catalog. A list of astronomical catalogues can be used to find which catalog a star or other object is from based on its prefix. Most objects are listed in several catalogs and will often be known by several different designations.
Observation
HE 1523-0901 is approximately 27 solar masses, but the star has expanded until it is some 730 times as large, and has a total luminosity of 240,000 times that of the Sun. It can be viewed particularly well from the southern hemisphere with the use of a small telescope. It can also be observed from central European latitudes.
See also
References
- ^ a b c d e f g h Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b Beers, Timothy C.; Flynn, Chris; Rossi, Silvia; Sommer-Larsen, Jesper; Wilhelm, Ronald; Marsteller, Brian; Lee, Young Sun; De Lee, Nathan; Krugler, Julie; Deliyannis, Constantine P.; Simmons, Andrew T.; Mills, Elisabeth; Zickgraf, Franz-Josef; Holmberg, Johan; Önehag, Anna; Eriksson, Anders; Terndrup, Donald M.; Salim, Samir; Andersen, Johannes; Nordström, Birgitta; Christlieb, Norbert; Frebel, Anna; Rhee, Jaehyon (2007). "Broadband UBVRCIC Photometry of Horizontal-Branch and Metal-poor Candidates from the HK and Hamburg/ESO Surveys. I.". The Astrophysical Journal Supplement Series. 168 (1): 128. arXiv:astro-ph/0610018. Bibcode:2007ApJS..168..128B. doi:10.1086/509324. S2CID 119500060.
- ^ Placco, Vinicius M.; Beers, Timothy C.; Santucci, Rafael M.; Chanamé, Julio; Sepúlveda, María Paz; Coronado, Johanna; Points, Sean D.; Kaleida, Catherine C.; Rossi, Silvia; Kordopatis, Georges; Lee, Young Sun; Matijevič, Gal; Frebel, Anna; Hansen, Terese T.; Holmbeck, Erika M.; Rasmussen, Kaitlin C.; Roederer, Ian U.; Sakari, Charli M.; Whitten, Devin D. (2018). "Spectroscopic Validation of Low-metallicity Stars from RAVE". The Astronomical Journal. 155 (6): 256. arXiv:1805.00608. Bibcode:2018AJ....155..256P. doi:10.3847/1538-3881/aac20c. S2CID 119460225.
- ^ a b c d Reggiani, Henrique; Ji, Alexander P.; Schlaufman, Kevin C.; Frebel, Anna; Necib, Lina; Nelson, Tyler; Hawkins, Keith; Galarza, Jhon Yana (2022). "The Chemical Composition of Extreme-velocity Stars". The Astronomical Journal. 163 (6): 252. arXiv:2203.16364. Bibcode:2022AJ....163..252R. doi:10.3847/1538-3881/ac62d9. S2CID 247793231.
- ^ a b c Frebel, A.; et al. (2007). "Discovery of HE 1523–0901, a Strongly r-Process-enhanced Metal-poor Star with Detected Uranium". The Astrophysical Journal. 660 (2): L117. arXiv:astro-ph/0703414. Bibcode:2007ApJ...660L.117F. doi:10.1086/518122. S2CID 17533424.
- ^ "Nearby Star Is A Galactic Fossil". Science Daily. May 11, 2007. Retrieved 2007-05-10.
- ^ "A galactic fossil: Star is found to be 13.2 billion years old". PhysOrg. May 10, 2007. Retrieved 2007-05-12.
External links
- "Astronomers discover HE 1523-0901 star: Almost as old as universe". iTWire. Archived from the original on 2007-05-14. Retrieved 2007-05-15.
- "Ancient star nearly as old as the universe". NBC News. 11 May 2007. Retrieved 2007-05-14.
